Skip to main content

Spitzer’s View of NGC2264’s Circumstellar Disk Population

  • Conference paper
  • First Online:

Part of the book series: Astrophysics and Space Science Proceedings ((ASSSP))

Abstract

We present a Spitzer study of the pre-main sequence population of the young cluster NGC 2264. The disk population is divided into three classes, based on individual spectral energy distributions: optically thick disks, in a homologous manner depleted or anemic disks, and radially depleted transition disks. Our analysis indicated that there may be two distinct evolutionary paths; disks evolve from optically thick to anemic via the first path, and from optically thick to transition in the second. Most of the disks seem to follow the first path. It is yet unknown what physical mechanism triggers this evolutionary differentiation – it could be directly connected to the nature of planet formation within the disk.

This is a preview of subscription content, log in via an institution.

Buying options

Chapter
USD   29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD   129.00
Price excludes VAT (USA)
  • Available as EPUB and PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD   169.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info
Hardcover Book
USD   169.99
Price excludes VAT (USA)
  • Durable hardcover edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Learn about institutional subscriptions

References

  1. Butler, R.P., et al.: Astrophys. J. 646, 505 (2006)

    Article  ADS  Google Scholar 

  2. Dahm, S.E.: Handbook of Star Forming Regions, vol. I, 966. San Francisco, CA: ASP (2008)

    Google Scholar 

  3. Lada, C.J., Lada, E.A.: Annu. Rev. Astron. Astrophys. 41, 57 (2003)

    Article  ADS  Google Scholar 

  4. Lada, C.J., et al.: Astron. J. 131, 1574 (2006)

    Article  ADS  Google Scholar 

  5. Teixeira, P.S., et al.: Astrophys. J. Lett. 636, L45 (2006)

    Article  ADS  Google Scholar 

  6. Teixeira, P.: Ph.D. Thesis, Universidade de Lisboa, Portugal (2008)

    Google Scholar 

  7. Teixeira, P.S., Lada, C.J., Marengo, M., Lada, E.A.: Astron. Astrophys.(submitted) (2010)

    Google Scholar 

  8. Walker, M.F.: Astrophys. J. Suppl. 2, 365 (1956)

    Article  ADS  Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to Paula S. Teixeira .

Editor information

Editors and Affiliations

Rights and permissions

Reprints and permissions

Copyright information

© 2012 Springer-Verlag Berlin Heidelberg

About this paper

Cite this paper

Teixeira, P.S., Lada, C.J., Marengo, M., Lada, E. (2012). Spitzer’s View of NGC2264’s Circumstellar Disk Population. In: Moitinho, A., Alves, J. (eds) Star Clusters in the Era of Large Surveys. Astrophysics and Space Science Proceedings. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-22113-2_45

Download citation

  • DOI: https://doi.org/10.1007/978-3-642-22113-2_45

  • Published:

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-642-22112-5

  • Online ISBN: 978-3-642-22113-2

  • eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)

Publish with us

Policies and ethics